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Parameter Estimation of Pulsar Position Based on Least Square

机译:基于最小二乘法的脉冲星位置参数估计

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The pulsar position parameters error is one of the main factors affecting the accuracy of X-ray pulsar autonomous navigation and pulsar time keeping. There is a nonlinear relationship between pulsar position parameters and pulsar timing residuals. Based on the above issues, this paper established a mathematical model for parameter estimation of pulsars' right ascension and declination errors, analyzed the pulsar timing residuals caused by different planetary ephemeris, and studied the influence of the errors of right ascension and declination of pulsars on the timing residuals. On this basis, the pulsar position parameters are estimated by the least square method. And the simulation experiment and analysis are carried out. The results show that, based on the proposed method, using DE430 planetary ephemeris. when the timing residual is 0.1 us, the accuracy of pulsar position estimation accuracy is about 0.03 mas, which shows the effectiveness of the proposed method.
机译:脉冲星位置参数误差是影响X射线脉冲星自主导航和脉冲星时间保持精度的主要因素之一。脉冲星位置参数与脉冲星定时残差之间存在非线性关系。基于上述问题,本文建立了脉冲星赤经误差参数估计的数学模型,分析了不同星历引起的脉冲星时间残差,研究了脉冲星赤经误差对时间残差的影响。在此基础上,利用最小二乘法对脉冲星位置参数进行了估计。并进行了仿真实验和分析。结果表明,基于该方法,使用DE430行星历。当时间残差为0.1us时,脉冲星位置估计精度约为0.03mas,表明了该方法的有效性。

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